High Redshift Starbursts Mauro Giavalisco Space Telescope Science Institute and the GOODS team STScI/ESO/ST-ECF/JPL/SSC/Gemini/Boston U./U. Ariz./U. Fla./U.
Deblending issues working report MontePorzio 16-04-08 CU5#DU11 Luigi Pulone@ INAF-OA Roma INAF - Teramo Observatory: Anna Piersimoni, Giorgia Busso INAF.
Solar system
Hydrogen Burning and Pulsations on Low Mass Helium Core White Dwarfs Justin D. R. Steinfadt Lars Bildsten UCSB Wild Stars in the Wild West II 14th North.
Early accreting SMBHs: forecasts for the next decade with the Wide Field X-ray Telescope R. Gilli (INAF-OABo), P. Tozzi, P. Rosati, S. Borgani, M. Paolillo,
The Milky Way. The Milky Way: Our Home Galaxy What are the different components of the Milky Way? How do we see those components? What does a map of each.
Distance Determination of the Hubble Constant H o by the use of Parallax and Cepheid Variable Stars presented by Michael McElwain and G. Richard Murphy.
The Galactic Habitable Zone Guillermo Gonzalez Iowa State University Fermilab August 21, 2002 Acknowledgements: Don Brownlee Peter Ward.
1 THE LOCAL HIGH REDSHIFT UNIVERSE – THE EXTREMELY METAL POOR STARS IN THE GALACTIC HALO Why study very metal poor stars ? We can study the early epochs.
John Bally
Three-dimensional hydrodynamical simulations of ISM pollution by type Ia and II supernovae in forming dwarf spheroidal galaxies Andrea Marcolini (Bologna.
IZI: INFERRING METALLICITIES AND IONIZATION PARAMETERS WITH BAYESIAN STATISTICS Guillermo A. Blanc Universidad de Chile.
